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- Currently displaying 381 - 400 of 2092 publications
Salvete
– SEISMOLOGY OF THE SUN AND THE DISTANT STARS 2016-USING TODAY'S SUCCESSES TO PREPARE THE FUTURE
(2017)
160,
00003
(doi: 10.1051/epjconf/201716000003)
A fitting LEGACY - Modelling Kepler 's best stars
– SEISMOLOGY OF THE SUN AND THE DISTANT STARS 2016-USING TODAY'S SUCCESSES TO PREPARE THE FUTURE
(2017)
160,
03010
(doi: 10.1051/epjconf/201716003010)
Gravito-turbulence and the excitation of small-scale parametric instability in astrophysical discs
– Monthly Notices of the Royal Astronomical Society
(2017)
471,
317
(doi: 10.1093/mnras/stx1548)
The degree of knottedness of tangled vortex lines – CORRIGENDUM
– Journal of Fluid Mechanics
(2017)
830,
821
(doi: 10.1017/jfm.2017.667)
On Multi-Level Thinking and Scientific Understanding
– Advances in Atmospheric Sciences
(2017)
34,
1150
(doi: 10.1007/s00376-017-6283-3)
Cool and hot emission in a recurring active region jet
– Astronomy & Astrophysics
(2017)
606,
A4
(doi: 10.1051/0004-6361/201730429)
Magnetorotational instability and dynamo action in gravito-turbulent astrophysical discs
– Monthly Notices of the Royal Astronomical Society
(2017)
474,
2212
(doi: 10.1093/mnras/stx2455)
In situ accretion of gaseous envelopes on to planetary cores embedded in evolving protoplanetary discs
– Monthly Notices of the Royal Astronomical Society
(2017)
470,
3206
(doi: 10.1093/mnras/stx1297)
Dynamical tides in exoplanetary systems containing hot Jupiters: confronting theory and observations
– Monthly Notices of the Royal Astronomical Society
(2017)
470,
2054
(doi: 10.1093/mnras/stx1234)
Non-axisymmetric instabilities in discs with imposed zonal flows
(2017)
(doi: 10.48550/arxiv.1609.02459)
Spectroscopy of Very Hot Plasma in Non-flaring Parts of a Solar Limb Active Region: Spatial and Temporal Properties
– The Astrophysical Journal
(2017)
846,
25
(doi: 10.3847/1538-4357/aa835f)
Amplification of Magnetic Fields by Compressible Convection
– Symposium - International Astronomical Union
(2017)
102,
301
(doi: 10.1017/s0074180900029958)
Do solar models with weakly interacting massive particles reproduce the Stanford seismic data?
– Symposium - International Astronomical Union
(2017)
123,
111
(doi: 10.1017/s0074180900157857)
Solar equatorial rotation rate inferred from inversion of frequency splitting of high-degree modes
– Symposium - International Astronomical Union
(2017)
123,
45
(doi: 10.1017/s0074180900157705)
The magnetic local time distribution of energetic electrons in the radiation belt region
– Journal of Geophysical Research Space Physics
(2017)
122,
8108
(doi: 10.1002/2017ja024084)
ON THE EXCITATION OF SOLAR 5-MINUTE OSCILLATIONS
– Symposium - International Astronomical Union
(2017)
123,
371
(doi: 10.1017/s0074180900158371)
Magnetic perturbations to stellar oscillation eigenfrequencies
– Symposium - International Astronomical Union
(2017)
123,
155
(doi: 10.1017/s0074180900157973)
Helium diffusion in rapidly oscillating Ap stars
– Symposium - International Astronomical Union
(2017)
123,
291
(doi: 10.1017/s0074180900158267)
On the implications of the symmetric component of the frequency splitting reported by Duvall, Harvey and Pomerantz
– Symposium - International Astronomical Union
(2017)
123,
175
(doi: 10.1017/s0074180900158012)